Fourth of July is the perfect time to watch fiery masses streak across the sky. This speedy guy, the comet ISON, looks like it pretty much fits that bill. Except that it’s actually quite icy at its core, and it’s barreling toward the sun at around 48,000 miles per hour, faster than any firework.

This five-second loop of video is a compression of images taken by the Hubble Space Telescope over a period of 43 minutes in May, during which ISON covered 34,000 miles.

The Ring Nebula New images of the Ring Nebula captured by the Hubble Space Telescope are redefining the way astronomers understand its shape. NASA, ESA, C.R. Robert O’Dell (Vanderbilt University), G.J. Ferland (University of Kentucky), W.J. Henney and M. Peimbert (National Autonomous University of Mexico)

The Universe’s first galaxies played a key role in shaping the environment in which we now find ourselves. They fostered the formation of the first stars, which died in spectacular explosions that enabled a new generation of smaller stars, orbited by rockier planets. And the galaxies themselves merged and grew, forming the large galaxies and clusters that populate the Universe today. But, despite their critical role in shaping the Universe, we’ve never actually been able to see one of them.

Slowly, that’s changing. The Hubble Deep Field exposures have helped us spot galaxies from the Universe’s early days. But now, a special Hubble project has used an intervening cluster of galaxies as a lens to spot what appears to be the most distant galaxy ever imaged, one that dates from just 425 million years after the Big Bang.

Since it takes light time to reach us from distant corners of the Universe, the further you look, the older the objects you see. The wavelength of the light also gets shifted towards the red by the expansion of the Universe, which stretches it out as it travels. As you get closer to the Big Bang, light that started out in the UV end of the spectrum gets pushed deeper and deeper into the infrared. To make these galaxies even harder to spot, the extreme distance means that very few photons actually make their way to Earth, so these objects are incredibly dim.

The name of this thing is AFGL 3068. It’s been known as a bright infrared source for some time, but images just showed it as a dot. This Hubble image using the Advanced Camera for Surveys reveals an intricate, delicate and exceedingly faint spiral pattern. It’s so faint no one has ever detected it before!

So what’s going on here? First off, this is not a spiral galaxy! It’s a binary star*, two stars that orbit each other, located about 3000 light years away from us. One of the stars is what’s called a carbon star, similar to the Sun but much older. The Sun is still happily fusing hydrogen into helium in its core, but older stars run out of available hydrogen. Eventually, they fuse helium into carbon. When this happens the star swells up and becomes a red giant (note: that’s the brief version; the actual events are a tad more complicated).

This image snapped by the NASA/ESA Hubble Space Telescope reveals an exquisitely detailed view of part of the disc of the spiral galaxy NGC 4565. This bright galaxy is one of the most famous examples of an edge-on spiral galaxy, oriented perpendicularly to our line of sight so that we see right into its luminous disc. NGC 4565 has been nicknamed the Needle Galaxy because, when seen in full, it appears as a very narrow streak of light on the sky.

The edgewise view into the Needle Galaxy shown here looks very similar to the view we have from our Solar System into the core of the Milky Way. In both cases ribbons of dust block some of the light coming from the galactic disc. To the lower right, the dust stands in even starker contrast against the copious yellow light from the star-filled central regions. NGC 4565’s core is off camera to the lower right.

ScienceDaily (July 11, 2012) — A team of astronomers using NASA’s Hubble Space Telescope is reporting the discovery of another moon orbiting the icy dwarf planet Pluto.

This image, taken by NASA’s Hubble Space Telescope, shows five moons orbiting the distant, icy dwarf planet Pluto. The green circle marks the newly discovered moon, designated P5, as photographed by Hubble’s Wide Field Camera 3 on July 7. The observations will help scientists in their planning for the July 2015 flyby of Pluto by NASA’s New Horizons spacecraft. P4 was uncovered in Hubble imagery in 2011. (Credit: NASA; ESA; M. Showalter, SETI Institute)

The moon is estimated to be irregular in shape and 6 to 15 miles across. It is in a 58,000-mile-diameter circular orbit around Pluto that is assumed to be co-planar with the other satellites in the system.

“The moons form a series of neatly nested orbits, a bit like Russian dolls,” said team lead Mark Showalter of the SETI Institute in Mountain View, Calif.

The discovery increases the number of known moons orbiting Pluto to five.

The Pluto team is intrigued that such a small planet can have such a complex collection of satellites. The new discovery provides additional clues for unraveling how the Pluto system formed and evolved. The favored theory is that all the moons are relics of a collision between Pluto and another large Kuiper belt object billions of years ago.